Why Fast-Spinning Young Stars Don't Fly Apart

Why Fast-Spinning Young Stars Don't Fly Apart
A developing star is collapsing onto itself at top-left in this artist's conception. As it shrinks, the star spins faster and faster, like a skater folding in his or her arms. Green lines represent magnetic fields. Leftover material forms a flat disk, in which the magnetic field gets bogged down. (Image credit: NASA/JPL-Caltech/R. Hurt (SSC))

Young stars are loaded with energy, and they can spin around in half a day or less, compared to the 28 days it takes our more mature Sun to make a revolution.

But young stars would spin even faster if something didn't hold them back.

Now scientists say they think they've figured out at least one thing that slows them down: disks of planet-forming gas and dust, just as had been long suspected.

Developing stars spin so fast that, left unchecked, they would never fully contract and become stars. A disk tugs at a star's magnetic field, something like a spoon moving through molasses, the researchers said.

The support for this scenario, announced today, is based on new observations from NASA's Spitzer Space Telescope, which found that slow-spinning stars are five times as likely to have a disk as fast spinners.

"We can now say that disks play some kind of role in slowing down stars in at least one region, but there could be a host of other factors operating in tandem," said study leader Luisa Rebull of NASA's Spitzer Science Center. "And stars might behave differently in different environments."

Other factors that contribute to a star's winding down over longer periods of time include stellar winds and possibly full-grown planets.

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